X-ray reverberation modelling of the observed UV/optical power spectra of quasars

Open Access

Table 1.

Parameter values for which we computed the model power spectra.

Parameter		Values
Wavelength	λ_rest (Å)	1300, 1800, 2300, 3000, 3400, 4000
BH mass, accretion rate, redshift	( $log M_{BH}, {\dot{m}}_{Edd}, \bar{z})$ $\log M_{\mathrm{BH}}, \dot{m}_{\mathrm{Edd}}, \overline{z})$	(8.3, 0.1, 0.72), (8.3, 0.2, 1.04), (8.3, 0.4, 1.43)
		(8.9, 0.04, 1.03), (8.9, 0.1, 1.44), (8.9, 0.25, 1.77)
		(9.5, 0.025, 1.44), (9.5, 0.05, 1.88), (9.5, 0.1, 1.82)
X-ray luminosity	L_transf/L_disc
(when corona is powered by the accretion process)		0.1, 0.3, 0.5, 0.7, 0.9
(when corona is powered an external source)		−1.9, −1.7, ..., −0.3, −0.1
Corona height	h (R_g)	2.5, 5, 10, 20, ..., 90
Colour-correction factor	f_col	1, 1.7, 2.5
BH spin	α^*	0, 0.7, 0.998

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